Orbital patterns refer to the paths that celestial bodies, such as planets and moons, follow as they move around larger objects like stars or planets. These paths are typically elliptical, meaning they are shaped like elongated circles. The gravitational pull of the larger object keeps the smaller body in orbit, balancing the forces of attraction and inertia. The most well-known example of orbital patterns is the Earth's orbit around the Sun. This orbit takes about 365 days to complete, resulting in the changing seasons. Other celestial bodies, like the Moon, also have their own orbital patterns, revolving around the Earth approximately every 27.3 days.